Exam 19: Origin of the Solar System and Extrasolar Planets

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Almost every solid surface in the Solar System is covered with _______________, most of which formed during a period of heavy bombardment.

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Which hypothesis was out-ruled by the solar nebular theory?

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In the inner solar nebula, only metals and silicates could form solids, so the _______________ planets grew slowly.

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What astronomical object is the most important source for determining the age of our Solar System?

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The Jovian planets formed beyond the _______________, where water vapor, methane, and ammonia could freeze to form ice particles.

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The first extrasolar planets discovered are small and have long orbital periods.

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From meteorite and lunar rock samples, astronomers have determined the age of the Solar System to be ____.

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Water vapor, methane, and ammonia were abundant in the solar nebula.

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Laplace's nebular hypothesis was problematic in that he could not explain ____.

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Which physical property in Laplace's nebular hypothesis could not explain the Sun's slow rotation?

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Asteroids are the last of the icy planetesimals from the formation of the Solar System.

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Georges-Louis de Buffon was the first to propose that the Sun and planets formed when a large vortex contracted and condensed.

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Which theory best describes today's current thinking about the birth of a solar system?

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Which best describes the appearance of an asteroid?

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The inner planets are composed of rock and metal, and the outer planets are rich in low-density gases such as hydrogen and helium.

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During Solar System formation, solid particles contracted from the gas of the nebula as it cooled.

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Planetesimals beyond the orbit of _____ failed to accumulate into a protoplanet because the gravitational field of _____ continuously disturbed their motion.

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What are the small bits of rock and metal that collide with Earth's atmosphere?

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According to the solar nebula theory, Earth and the other planets of the Solar System formed billions of years ago as the Sun _______________ from a cloud of interstellar gas and dust.

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The dense disks of gas and dust such as those seen around the stars in Orion are sites where planets could be forming right now.

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